EE Cam is a previously little studied Delta Scuti pulsator with amplitudes between those of the HADS ( High-Amplitude Delta Scuti stars ) group and the average low-amplitude pulsators . Since the size of stellar rotation determines both which pulsation modes are selected by the star as well as their amplitudes , the star offers a great opportunity to examine the astrophysical connections . Extensive photometric measurements covering several months were carried out . 15 significant pulsation frequencies were extracted . The dominant mode at 4.934 cd ^ { -1 } was identified as a radial mode by examining the phase shifts at different wavelengths . Medium-dispersion spectra yielded a v \sin i value of 40 \pm 3 km s ^ { -1 } . This shows that EE Cam belongs to the important transition region between the HADS and normal Delta Scuti stars .